Chandrasekhar leemit

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The Chandrasekhar leemit is the maximum mass o a stable white dwarf starn. The leemit wis first indicatit in papers published bi Wilhelm Anderson an E. C. Stoner, an wis named efter Subrahmanyan Chandrasekhar, the Indian astropheesicist wha independently discovered an improved upon the accuracy o the calculation in 1930, at the age o 19, in Indie.